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F & H Solar Radio Emission: Delayed Fundamental

Published online by Cambridge University Press:  14 August 2015

Anthony Achong
Anthony Achong*
Affiliation:
Department of Physics, University of the West Indies, St. Augustine, Trinidad, W.I.

Abstract

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The suggestion is made that the excessive time delays between the two components of f-h type III pairs might be partly accounted for by an initial production of the second harmonic only, followed later by the production of both components. The source is assumed to be inside coronal streamers. Theoretical arguments lend some support to the suggestion of a delayed start of the fundamental.

Type
Session V - Solar Bursts - Meter-Decameter Wavelengths
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 323 - 325
Copyright
Copyright © Reidel 1980 

References

Alvarez, H., and Haddock, F.T.: Solar Phys., 29(1973) pp 197–209.Google Scholar
Caroubalos, C., Poquerusse, M., and Steinberg, J.L.: Astron. Astrophys. 32 (1974) pp 255–267.Google Scholar
Daigne, G., and Møller-Pedersen, B.: Astron. Astrophys. 37 (1974) pp 355.Google Scholar
Haddock, F.T., and Alvarez, H.: Solar Phys. 29 (1973) pp 183–196.Google Scholar
Hughes, M.P., and Harkness, R.L.: Astrophys. J. 138 (1963) pp 239.Google Scholar
Newkirk, G.: Astrophys. J. 133 (1961) pp 983–1013.CrossRefGoogle Scholar
Smith, D.F.: Space Sc. Rev. 16 (1974) pp 91–144.Google Scholar